共查询到20条相似文献,搜索用时 188 毫秒
1.
2.
3.
航天器密封舱在地面模拟试验中常通过降压法抑制自然对流的影响,但降压比的选择 往往缺乏定量准则,这使得自然对流的抑制效果得不到保证。使用数值模拟方法确定临 界压力比,以几种典型航天器密封舱内的流动换热情况为例,分析了不同Gr/Re 2 数和压力比下密封舱内的流动换热情况。得到了舱内气体温度分布和对流换热系数。通 过比较空间情况和地面情况的计算结果,分析了自然对流给流动换热带来的影响,给出了判 断临界压力的准则式,并给出了临界Gr/Re 2数。结果表明:临界压力 的准则关系和密封舱的形状和内部结构无关。
相似文献
相似文献
4.
通过对常用的大气压累积法氦质谱检漏过程的理论分析,指出了该方法可能的系统误差。分析认为:对于表面材料粘附几率较小的被检件,可以采用常用的大气压累积检漏方法进行总漏率的测量,而对于表面材料粘附几率较大的被检件( 如表面存在大量的有机材料等) ,如采用常用的大气压累积检漏方法进行总漏率的测量必将带来较大的系统误差。最后,提出了消除该系统误差的等分压常压累积检漏技术,并与常用的常压累积法检漏技术进行了比较。 相似文献
5.
M.A. Kolosov O.I. Yakovlev A.I. Efimov S.S. Matyugov T.S. Timofeeva E.V. Chub A.G. Pavelyev A.I. Kucheryavenkov I.E. Kalashnikov O.E. Milekhin 《Acta Astronautica》1980,7(2):219-234
Using the Venera-9 and 10 satellites radio occultation measurements of the atmosphere and bistatic radar measurements of the surface of the planet Venus were realized from October 1975 to March 1976. The altitude dependence of the molecular number density, pressure and temperature on the night and day sides were derived.An analysis is made of the stratified structure and turbulence in the atmosphere of Venus. The results of pressure measurements on the surface by the method of bistatic radar are presented. The diagrams and the tables of the parameters of the atmosphere are given. 相似文献
6.
针对工作在高真空环境下的轨控发动机,数值模拟了其羽流红外特性。首先计算了考虑化学反应的轨控发动机喷管的内流场和外流场,得到了温度、压力、组分浓度等参数的分布。基于HITRAN 2008和HITEMP 2010数据库采用逐线积分法编程计算了气体光谱吸收系数。最后在此基础上用有限体积法建立的求解辐射传输方程的模型,计算得到羽流红外辐射强度在2~10μm范围内随波长变化的曲线。分析了羽流气体组分、波长、探测角度对羽流光谱辐射的影响,与同类文献中的计算结果进行了比较,结果表明:本文的计算模型和方法能较好地模拟轨控发动机羽流的红外辐射特性。 相似文献
7.
真空室压升法测量液态工质漏率可行性分析 总被引:1,自引:1,他引:0
文章旨在探讨压升法测量液态工质漏率的可行性,研究液体泄漏的试验方法。首先根据液体饱和蒸气压的理论分析,得出液体挥发引起的定容压力增量;之后通过微进样系统,采用真空室静态升压方法,分别以全氟三乙胺和乙二醇水溶液为研究对象进行试验分析,研究得出漏入液体量V与压力变化ΔP成线性关系,与理论分析计算结果相符合,证明了压升法测液态工质漏率的可行性;最后提出了微量采样系统进行比对测量液态工质漏率的压升试验方法及计算公式。研究结果表明,压升法可有效地测量液态工质漏率,为液体的流动试验研究提供参考依据。 相似文献
8.
9.
《Acta Astronautica》2007,60(10-11):880-888
The Korea Sounding Rocket-III (KSR-III) was successfully launched on November 28, 2002 from the west coast of the Korean Peninsula. The science payload onboard the KSR-III included an ozone detector and two magnetometers along with other various sensors installed to measure physical characteristics such as temperature, pressure, strain, and acceleration. The main objective of KSR-III was to evaluate the liquid propulsion engine system which has been newly adopted in the KSR series. In addition to this main objective, the science payload conducted atmospheric soundings. The payload data were transmitted to the ground station in real time by an onboard telemetry system. The UV radiometer measured the direct solar UV radiation and during the ascending phase the vertical ozone density profile was obtained. This result was compared with coincident measurements taken by other satellites, a ground station, and an ozonesonde. A fluxgate-type magnetometer was onboard the KSR-III to observe the Earth's DC magnetic field and for AC field measurements, a search-coil magnetometer was installed. This was the first Korean mission to use magnetometers on a rocket-borne platform to measure the Earth's magnetic field. Using the telemetry magnetometer data, a study on the rocket attitude was carried out. This paper will give an overview of the design, calibration, and test results of the science payload onboard the KSR-III. 相似文献
10.
A method for determination of internal gravity wave (IGW) parameters from a single vertical temperature or density profile
measurement in the Earth’s atmosphere has been developed. This method may be used for the analysis of profiles measured by
any techniques in which the accuracy is enough to measure small (∼1%) amplitudes of the temperature or density fluctuations
in the atmosphere. The criterion for the IGW identification has been formulated and argued. In the case when this criterion
is satisfied then analyzed fluctuations can be considered as wave-induced. The method is based upon the analysis of relative
amplitude thresholds of the temperature or density wave field and upon linear IGW saturation theory in which amplitude thresholds
are restricted by dynamical instability processes in the atmosphere. In order to approbate the method we have used data of
simultaneous radiosonde measurements of the temperature and wind velocity in the Earth’s stratosphere where the saturated
IGW propagation has been detected. It is shown that the application of the method to radio occultation temperature data gives
the possibility to identify IGWs in the Earth’s lower stratosphere and to determine values of key wave parameters. 相似文献
11.
《Acta Astronautica》1987,15(11):945-949
This paper makes an attempt to offer a unification of the procedure of atmosphere corrections in remote sensing problems, using a Monte Carlo method for the calculations. 相似文献
12.
13.
为了给氧气/煤油发动机设计和热防护设计提供必要的设计参数,针对氧气/煤油燃气进行热力学计算。运用吉布斯最小自由焓计算模型得到燃气平衡组成,通过拟合公式的方法得到燃气的热物理参数及输运系数。通过计算,得到氧气/煤油燃气的组分及比焓、密度、比熵、粘性系数等热物理参数和输运系数随温度和压力的变化特性。分析结果表明:水离解对氧气/煤油燃气组分变化存在显著影响,压力增大会导致水离解起始温度升高;氧气/煤油燃气比焓、比熵、定压比热、粘性系数、热传导系数变化在温度较低时受压力影响较小,当水开始离解后,压力的影响显著增强;组分在燃气中的扩散系数同时受到了温度和组分摩尔分数的影响;燃气普朗特数变化受热传导系数变化的影响较大,水离解后,热传导系数的迅速增大使燃气的普朗特数迅速减小。 相似文献
14.
15.
多GNSS掩星大气探测卫星星座设计 总被引:1,自引:0,他引:1
为减少无线电掩星(RO)大气探测星座的卫星数量并增加探测数据量,将北斗(BD)和GPS、Galileo、GLONASS共同作为探测信源,提出一种多全球导航卫星系统(GNSS)掩星大气探测星座概念和优化设计方法。融合先验大气模型和二维射线追踪算法,建立兼容多GNSS信源的掩星事件前向模拟算法,实现掩星事件快速精确仿真;给出多GNSS掩星大气探测星座参数对探测性能的影响特性,降低了星座模型的复杂度;并利用改进的蚁群算法实现星座参数寻优。设计结果与COSMICII星座相比,卫星数量减少2颗,探测数据量增加了40%,探测均匀性提高了67%。 相似文献
16.
17.
18.
为了满足我国首次火星探测任务的需要,确保探测器有效载荷科学数据的顺利下传,将采用天线组阵的方式进行数据接收。天线组阵数据接收技术在航天工程中的应用国内尚属首次,为此开展了信号合成方法和处理流程的研究,提出了利用模型计算和基于科斯塔斯环的搜索估计相结合的初始时延和多普勒频差快速估计方法。利用现有的密云站50 m天线和昆明站40 m天线,以嫦娥3号着陆器数传信号为实验对象,开展了天线组阵与数据接收技术检验实验。研究和实验结果表明,全频谱合成方法优于符号流合成方法,其合成损耗小于等于 0.45 dB ,可用于我国首次火星探测任务天线组阵的信号合成;初始时延和多普勒频差快速估计方法可提高广域组阵信号互相关的搜索效率;所确定的信号合成技术流程和数据处理方法可用于后续信号合成软硬件设备的研制和开发。 相似文献
19.
电推进系统工质氙气充装特性试验研究 总被引:1,自引:1,他引:0
文章介绍了卫星电推进系统工质氙气充装特性试验系统及测试方法,开展了氙气充装饱和蒸气压,气相及超临界状态PVT充装特性试验研究,建立了新的氙气饱和蒸气压方程,拟合得到了氙气的临界压力,并与其他研究机构的试验数据进行了比较分析。氙气饱和蒸气压试验结果与NIST方程计算值的相对偏差小于0.2%,发现并验证了NIST方程计算值在近临界区的偏差最高达到6 kPa。试验数据为建立氙气充装加注预估模型奠定基础,为卫星电推进系统充装加注及在轨应用提供重要的参考。 相似文献
20.